Title

An efficient algorithm for determining positions of astronomical objects in the Deep Sky Object pictures

Journal title

Bulletin of the Polish Academy of Sciences Technical Sciences

Yearbook

2015

Volume

63

Issue

No 3

Authors

Suszynski, R. ; Wawryn, K. ; Dziebowski, M.

Divisions of PAS

Nauki Techniczne

Coverage

679-684

Date

2015[2015.01.01 AD - 2015.12.31 AD]

Identifier

DOI: 10.1515/bpasts-2015-0079 ; ISSN 2300-1917

Source

Bulletin of the Polish Academy of Sciences: Technical Sciences; 2015; 63; No 3; 679-684

References

Suszynski (2009), Convolution method for CCD images processing for DSO astrophotography nd Midwest Circuits and Systems, Proc IEEE Int Symp, 1. ; Suszynski (2011), image processing for auto - guiding system th Midwest on Circuits and Systems MWSCAS CD - ROM, Proc IEEE Int Symp, 1. ; Jeffs (1998), Blind bayesian restoration of adaptive optics telescope images using generalized gaussian markov random field models on Adaptive Optics and Telescope Systems SPIE CD - ROM, Proc Conf, 3353. ; McGuire (1998), Adaptive optics : neural networks wavefront sensing reconstruction and prediction th Seminar CD - ROM, Proc, 194. ; Vyas (2010), Cetroid detection by Gaussian pattern matching in adaptive optics Computer Applications, Int J, 1. ; Zhang (2012), Optical image simulation system for space surveillance th Parallel and Distributed Processing Symp CD - ROM, Proc IEEE Int. ; Li (2013), Implementing high - performance intensity model with blur effect on gpus for large - scale star image simulation on Image and Graphics CD - ROM, Proc Int Conf, 1. ; Berghi (2007), Atmospheric turbulence prediction : a pca approach th Decision and Control, Proc IEEE Conf, 1. ; Roesser (1975), A discrete state - space model for linear image processing, IEEE Trans Automat Contr, 20, 1, doi.org/10.1109/TAC.1975.1100844 ; Suszynski (2013), Rapid prototyping of algorithmic converters based on FPAA devices, Bull Pol Tech, 61, 691. ; Suszynski (2014), An improvement of stars centroid determination using PSF - fitting method Signals and Electronics Systems ICSES, Proc IEEE Int Conf, 1. ; Thomas (2006), Comparison of centroid computation algorithms in a Shack - Hartmann sensor Monthly Notices of the Royal, Astronomical Society, 371. ; Wawryn (2013), Low power bit pipelined - bit self - calibrated converters for a DSP system, Bull Pol Tech, 8, 979. ; Suszynski (2014), A stand - alone station and DSP method for deep sky objects astrophotography Electronics and Telecommunications, Int J, 157. ; Li (2006), The implement of high speed correlation tracking algorithm based on FPGA in space solar telescope th on Signal Processing CD - ROM, Proc Int Conf, 8, 1. ; Suszynski (2008), Digital processing of CCD images for auto - guiding astrophotography system th on Mixed Design of Integrated Circuits and Systems, Proc Int Conf, 15, 559. ; Baker (2007), Iteratively weighted centroid of Shack - Hartmann wave - front sensors, Opt Express, 15, 5147, doi.org/10.1364/OE.15.005147 ; Suszynski (2009), Stand - alone station for deep space objects astrophotography nd Midwest Symposium on Circuits and Systems, Proc IEEE Int, 1. ; Wawryn (2010), Implementation of finite impulse response systems using rotation structures Information Theory and Its Applications ISITA CD - ROM, Proc Int Symp, 20101.